DipoleMeasurementTask¶
- class lsst.ip.diffim.DipoleMeasurementTask(schema, algMetadata=None, **kwds)¶
Bases:
SingleFrameMeasurementTask
Measurement of Sources, specifically ones from difference images, for characterization as dipoles
- Parameters:
Notes
The list of badFlags will be used to make a list of keys to check for measurement flags on. By default the centroid keys are added to this list
Description
This class provides a default configuration for running Source measurement on image differences.
class DipoleMeasurementConfig(SingleFrameMeasurementConfig): "Measurement of detected diaSources as dipoles" def setDefaults(self): SingleFrameMeasurementConfig.setDefaults(self) self.plugins = ["base_CircularApertureFlux", "base_PixelFlags", "base_SkyCoord", "base_PsfFlux", "ip_diffim_NaiveDipoleCentroid", "ip_diffim_NaiveDipoleFlux", "ip_diffim_PsfDipoleFlux", "ip_diffim_ClassificationDipole", ] self.slots.calibFlux = None self.slots.modelFlux = None self.slots.instFlux = None self.slots.shape = None self.slots.centroid = "ip_diffim_NaiveDipoleCentroid" self.doReplaceWithNoise = False
These plugins enabled by default allow the user to test the hypothesis that the Source is a dipole. This includes a set of measurements derived from intermediate base classes DipoleCentroidAlgorithm and DipoleFluxAlgorithm. Their respective algorithm control classes are defined in DipoleCentroidControl and DipoleFluxControl. Each centroid and flux measurement will have _neg (negative) and _pos (positive lobe) fields.
The first set of measurements uses a “naive” alrogithm for centroid and flux measurements, implemented in NaiveDipoleCentroidControl and NaiveDipoleFluxControl. The algorithm uses a naive 3x3 weighted moment around the nominal centroids of each peak in the Source Footprint. These algorithms fill the table fields ip_diffim_NaiveDipoleCentroid* and ip_diffim_NaiveDipoleFlux*
The second set of measurements undertakes a joint-Psf model on the negative and positive lobe simultaneously. This fit simultaneously solves for the negative and positive lobe centroids and fluxes using non-linear least squares minimization. The fields are stored in table elements ip_diffim_PsfDipoleFlux*.
Because this Task is just a config for SingleFrameMeasurementTask, the same result may be acheived by manually editing the config and running SingleFrameMeasurementTask. For example:
config = SingleFrameMeasurementConfig() config.plugins.names = ["base_PsfFlux", "ip_diffim_PsfDipoleFlux", "ip_diffim_NaiveDipoleFlux", "ip_diffim_NaiveDipoleCentroid", "ip_diffim_ClassificationDipole", "base_CircularApertureFlux", "base_SkyCoord"] config.slots.calibFlux = None config.slots.modelFlux = None config.slots.instFlux = None config.slots.shape = None config.slots.centroid = "ip_diffim_NaiveDipoleCentroid" config.doReplaceWithNoise = False schema = afwTable.SourceTable.makeMinimalSchema() task = SingleFrameMeasurementTask(schema, config=config)-
Debug variables
The
lsst.pipe.base.cmdLineTask.CmdLineTask
command line task interface supports a flag-d/–debug to import debug.py from your PYTHONPATH. The relevant contents of debug.py for this Task include:import sys import lsstDebug def DebugInfo(name): di = lsstDebug.getInfo(name) if name == "lsst.ip.diffim.dipoleMeasurement": di.display = True # enable debug output di.maskTransparency = 90 # display mask transparency di.displayDiaSources = True # show exposure with dipole results return di lsstDebug.Info = DebugInfo lsstDebug.frame = 1 config.slots.calibFlux = None config.slots.modelFlux = None config.slots.gaussianFlux = None config.slots.shape = None config.slots.centroid = "ip_diffim_NaiveDipoleCentroid" config.doReplaceWithNoise = False
This code is dipoleMeasTask.py in the examples directory, and can be run as e.g.
examples/dipoleMeasTask.py examples/dipoleMeasTask.py --debug examples/dipoleMeasTask.py --debug --image /path/to/image.fits
Start the processing by parsing the command line, where the user has the option of enabling debugging output and/or sending their own image for demonstration (in case they have not downloaded the afwdata package).
if __name__ == "__main__": import argparse parser = argparse.ArgumentParser( description="Demonstrate the use of SourceDetectionTask and DipoleMeasurementTask") parser.add_argument('--debug', '-d', action="store_true", help="Load debug.py?", default=False) parser.add_argument("--image", "-i", help="User defined image", default=None) args = parser.parse_args() if args.debug: try: import debug debug.lsstDebug.frame = 2 except ImportError as e: print(e, file=sys.stderr) run(args)
The processing occurs in the run function. We first extract an exposure from disk or afwdata, displaying it if requested:
def run(args): exposure = loadData(args.image) if args.debug: afwDisplay.Display(frame=1).mtv(exposure)
Create a default source schema that we will append fields to as we add more algorithms:
schema = afwTable.SourceTable.makeMinimalSchema()
Create the detection and measurement Tasks, with some minor tweaking of their configs:
# Create the detection task config = SourceDetectionTask.ConfigClass() config.thresholdPolarity = "both" config.background.isNanSafe = True config.thresholdValue = 3 detectionTask = SourceDetectionTask(config=config, schema=schema) # And the measurement Task config = DipoleMeasurementTask.ConfigClass() config.plugins.names.remove('base_SkyCoord') algMetadata = dafBase.PropertyList() measureTask = DipoleMeasurementTask(schema, algMetadata, config=config)
Having fully initialied the schema, we create a Source table from it:
# Create the output table tab = afwTable.SourceTable.make(schema)
Run detection:
# Process the data results = detectionTask.run(tab, exposure)
Because we are looking for dipoles, we need to merge the positive and negative detections:
# Merge the positve and negative sources fpSet = results.fpSets.positive growFootprint = 2 fpSet.merge(results.fpSets.negative, growFootprint, growFootprint, False) diaSources = afwTable.SourceCatalog(tab) fpSet.makeSources(diaSources) print("Merged %s Sources into %d diaSources (from %d +ve, %d -ve)" % (len(results.sources), len(diaSources), results.fpSets.numPos, results.fpSets.numNeg))
Finally, perform measurement (both standard and dipole-specialized) on the merged sources:
measureTask.run(diaSources, exposure)
Optionally display debugging information:
# Display dipoles if debug enabled if args.debug: dpa = DipoleAnalysis() dpa.displayDipoles(exposure, diaSources)
Attributes Summary
Name by which the noise exposire ID is recorded in metadata ('str').
Name by which the noise offset is recorded in metadata ('str').
Name by which the noise seed multiplier is recorded in metadata ('str').
Name by which the noise source is recorded in metadata ('str').
Metadata about active plugins (
lsst.daf.base.PropertyList
).Plugins to be invoked (
PluginMap
).Methods Summary
callMeasure
(measRecord, *args, **kwds)Call
measure
on all plugins and consistently handle exceptions.callMeasureN
(measCat, *args, **kwds)Call
measureN
on all plugins and consistently handle exceptions.doMeasurement
(plugin, measRecord, *args, **kwds)Call
measure
on the specified plugin.doMeasurementN
(plugin, measCat, *args, **kwds)Call
measureN
on the specified plugin.Empty (clear) the metadata for this Task and all sub-Tasks.
Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict.
Get metadata for all tasks.
Get the task name as a hierarchical name including parent task names.
getName
()Get the name of the task.
Get the schemas generated by this task.
Get a dictionary of all tasks as a shallow copy.
initializePlugins
(**kwds)Initialize plugins (and slots) according to configuration.
makeField
(doc)Make a
lsst.pex.config.ConfigurableField
for this task.makeSubtask
(name, **keyArgs)Create a subtask as a new instance as the
name
attribute of this task.measure
(measCat, exposure)Backwards-compatibility alias for
run
.run
(measCat, exposure[, noiseImage, ...])Run single frame measurement over an exposure and source catalog.
runPlugins
(noiseReplacer, measCat, exposure)Call the configured measument plugins on an image.
timer
(name[, logLevel])Context manager to log performance data for an arbitrary block of code.
Attributes Documentation
- NOISE_EXPOSURE_ID = 'NOISE_EXPOSURE_ID'¶
Name by which the noise exposire ID is recorded in metadata (‘str’).
- NOISE_OFFSET = 'NOISE_OFFSET'¶
Name by which the noise offset is recorded in metadata (‘str’).
- NOISE_SEED_MULTIPLIER = 'NOISE_SEED_MULTIPLIER'¶
Name by which the noise seed multiplier is recorded in metadata (‘str’).
- NOISE_SOURCE = 'NOISE_SOURCE'¶
Name by which the noise source is recorded in metadata (‘str’).
- algMetadata = None¶
Metadata about active plugins (
lsst.daf.base.PropertyList
).Contains additional information about active plugins to be saved with the output catalog. Will be filled by subclasses.
- plugins = None¶
Plugins to be invoked (
PluginMap
).Initially empty, this will be populated as plugins are initialized. It should be considered read-only.
Methods Documentation
- callMeasure(measRecord, *args, **kwds)¶
Call
measure
on all plugins and consistently handle exceptions.- Parameters:
- measRecord
lsst.afw.table.SourceRecord
The record corresponding to the object being measured. Will be updated in-place with the results of measurement.
- *args
Positional arguments forwarded to
plugin.measure
- **kwds
Keyword arguments. Two are handled locally:
- beginOrder
int
Beginning execution order (inclusive). Measurements with
executionOrder
<beginOrder
are not executed.None
for no limit.- endOrder
int
Ending execution order (exclusive). Measurements with
executionOrder
>=endOrder
are not executed.None
for no limit.
Others are forwarded to
plugin.measure()
.- beginOrder
- measRecord
Notes
This method can be used with plugins that have different signatures; the only requirement is that
measRecord
be the first argument. Subsequent positional arguments and keyword arguments are forwarded directly to the plugin.This method should be considered “protected”: it is intended for use by derived classes, not users.
- callMeasureN(measCat, *args, **kwds)¶
Call
measureN
on all plugins and consistently handle exceptions.- Parameters:
- measCat
lsst.afw.table.SourceCatalog
Catalog containing only the records for the source family to be measured, and where outputs should be written.
- *args
Positional arguments forwarded to
plugin.measure()
- **kwds
Keyword arguments. Two are handled locally:
- beginOrder:
Beginning execution order (inclusive): Measurements with
executionOrder
<beginOrder
are not executed.None
for no limit.- endOrder:
Ending execution order (exclusive): measurements with
executionOrder
>=endOrder
are not executed.None
for nolimit
.
Others are are forwarded to
plugin.measure()
.
- measCat
Notes
This method can be used with plugins that have different signatures; the only requirement is that
measRecord
be the first argument. Subsequent positional arguments and keyword arguments are forwarded directly to the plugin.This method should be considered “protected”: it is intended for use by derived classes, not users.
- doMeasurement(plugin, measRecord, *args, **kwds)¶
Call
measure
on the specified plugin.Exceptions are handled in a consistent way.
- Parameters:
- pluginsubclass of
BasePlugin
Plugin that will be executed.
- measRecord
lsst.afw.table.SourceRecord
The record corresponding to the object being measured. Will be updated in-place with the results of measurement.
- *args
Positional arguments forwarded to
plugin.measure()
.- **kwds
Keyword arguments forwarded to
plugin.measure()
.
- pluginsubclass of
Notes
This method can be used with plugins that have different signatures; the only requirement is that
plugin
andmeasRecord
be the first two arguments. Subsequent positional arguments and keyword arguments are forwarded directly to the plugin.This method should be considered “protected”: it is intended for use by derived classes, not users.
- doMeasurementN(plugin, measCat, *args, **kwds)¶
Call
measureN
on the specified plugin.Exceptions are handled in a consistent way.
- Parameters:
- pluginsubclass of
BasePlugin
Plugin that will be executed.
- measCat
lsst.afw.table.SourceCatalog
Catalog containing only the records for the source family to be measured, and where outputs should be written.
- *args
Positional arguments forwarded to
plugin.measureN()
.- **kwds
Keyword arguments forwarded to
plugin.measureN()
.
- pluginsubclass of
Notes
This method can be used with plugins that have different signatures; the only requirement is that the
plugin
andmeasCat
be the first two arguments. Subsequent positional arguments and keyword arguments are forwarded directly to the plugin.This method should be considered “protected”: it is intended for use by derived classes, not users.
- getAllSchemaCatalogs() Dict[str, Any] ¶
Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict.
- Returns:
- schemacatalogs
dict
Keys are butler dataset type, values are a empty catalog (an instance of the appropriate
lsst.afw.table
Catalog type) for all tasks in the hierarchy, from the top-level task down through all subtasks.
- schemacatalogs
Notes
This method may be called on any task in the hierarchy; it will return the same answer, regardless.
The default implementation should always suffice. If your subtask uses schemas the override
Task.getSchemaCatalogs
, not this method.
- getFullMetadata() TaskMetadata ¶
Get metadata for all tasks.
- Returns:
- metadata
TaskMetadata
The keys are the full task name. Values are metadata for the top-level task and all subtasks, sub-subtasks, etc.
- metadata
Notes
The returned metadata includes timing information (if
@timer.timeMethod
is used) and any metadata set by the task. The name of each item consists of the full task name with.
replaced by:
, followed by.
and the name of the item, e.g.:topLevelTaskName:subtaskName:subsubtaskName.itemName
using
:
in the full task name disambiguates the rare situation that a task has a subtask and a metadata item with the same name.
- getFullName() str ¶
Get the task name as a hierarchical name including parent task names.
- Returns:
- fullName
str
The full name consists of the name of the parent task and each subtask separated by periods. For example:
The full name of top-level task “top” is simply “top”.
The full name of subtask “sub” of top-level task “top” is “top.sub”.
The full name of subtask “sub2” of subtask “sub” of top-level task “top” is “top.sub.sub2”.
- fullName
- getSchemaCatalogs() Dict[str, Any] ¶
Get the schemas generated by this task.
- Returns:
- schemaCatalogs
dict
Keys are butler dataset type, values are an empty catalog (an instance of the appropriate
lsst.afw.table
Catalog type) for this task.
- schemaCatalogs
See also
Task.getAllSchemaCatalogs
Notes
Warning
Subclasses that use schemas must override this method. The default implementation returns an empty dict.
This method may be called at any time after the Task is constructed, which means that all task schemas should be computed at construction time, not when data is actually processed. This reflects the philosophy that the schema should not depend on the data.
Returning catalogs rather than just schemas allows us to save e.g. slots for SourceCatalog as well.
- getTaskDict() Dict[str, ReferenceType[Task]] ¶
Get a dictionary of all tasks as a shallow copy.
- Returns:
- taskDict
dict
Dictionary containing full task name: task object for the top-level task and all subtasks, sub-subtasks, etc.
- taskDict
- initializePlugins(**kwds)¶
Initialize plugins (and slots) according to configuration.
- Parameters:
- **kwds
Keyword arguments forwarded directly to plugin constructors.
Notes
Derived class constructors should call this method to fill the
plugins
attribute and add corresponding output fields and slot aliases to the output schema.In addition to the attributes added by
BaseMeasurementTask.__init__
, aschema`
attribute holding the output schema must be present before this method is called.Keyword arguments are forwarded directly to plugin constructors, allowing derived classes to use plugins with different signatures.
- classmethod makeField(doc: str) ConfigurableField ¶
Make a
lsst.pex.config.ConfigurableField
for this task.- Parameters:
- doc
str
Help text for the field.
- doc
- Returns:
- configurableField
lsst.pex.config.ConfigurableField
A
ConfigurableField
for this task.
- configurableField
Examples
Provides a convenient way to specify this task is a subtask of another task.
Here is an example of use:
class OtherTaskConfig(lsst.pex.config.Config): aSubtask = ATaskClass.makeField("brief description of task")
- makeSubtask(name: str, **keyArgs: Any) None ¶
Create a subtask as a new instance as the
name
attribute of this task.- Parameters:
- name
str
Brief name of the subtask.
- keyArgs
Extra keyword arguments used to construct the task. The following arguments are automatically provided and cannot be overridden:
“config”.
“parentTask”.
- name
Notes
The subtask must be defined by
Task.config.name
, an instance ofConfigurableField
orRegistryField
.
- run(measCat, exposure, noiseImage=None, exposureId=None, beginOrder=None, endOrder=None)¶
Run single frame measurement over an exposure and source catalog.
- Parameters:
- measCat
lsst.afw.table.SourceCatalog
Catalog to be filled with the results of measurement. Must contain all the
lsst.afw.table.SourceRecord
s to be measured (withlsst.afw.detection.Footprint
s attached), and have a schema that is a superset ofself.schema
.- exposure
lsst.afw.image.ExposureF
Image containing the pixel data to be measured together with associated PSF, WCS, etc.
- noiseImage
lsst.afw.image.ImageF
, optional Can be used to specify the a predictable noise replacement field for testing purposes.
- exposureId
int
, optional Unique exposure identifier used to calculate the random number generator seed during noise replacement.
- beginOrder
float
, optional Start execution order (inclusive): measurements with
executionOrder < beginOrder
are not executed.None
for no limit.- endOrder
float
, optional Final execution order (exclusive): measurements with
executionOrder >= endOrder
are not executed.None
for no limit.
- measCat
- runPlugins(noiseReplacer, measCat, exposure, beginOrder=None, endOrder=None)¶
Call the configured measument plugins on an image.
- Parameters:
- noiseReplacer
NoiseReplacer
Used to fill sources not being measured with noise.
- measCat
lsst.afw.table.SourceCatalog
Catalog to be filled with the results of measurement. Must contain all the
lsst.afw.table.SourceRecord
s to be measured (withlsst.afw.detection.Footprint
s attached), and have a schema that is a superset ofself.schema
.- exposure
lsst.afw.image.ExposureF
Image containing the pixel data to be measured together with associated PSF, WCS, etc.
- beginOrder
float
, optional Start execution order (inclusive): measurements with
executionOrder < beginOrder
are not executed.None
for no limit.- endOrder
float
, optional Final execution order (exclusive): measurements with
executionOrder >= endOrder
are not executed.None
for no limit.
- noiseReplacer